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We model the binary black hole system OJ287 as a spinning primary and a non-spinning secondary.
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Ciprini, S. & Rizzi, N.: OJ287 colors during a multifrequency campaign. Proceedings of the Workshop on Blazar Variability across the Electromagnetic Spectrum, April 22-25, 2008, Palaiseau, France, published online at http://pos.sissa.it, p. 30-36 (2008)
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Sundelius, B., Wahde, M., Lehto, H.J. & Valtonen, M.J.: A numerical simulation of the brightness variations of OJ287. ApJ484, 180-185 (1997)
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Wu, J., Zhou, X., Wu, X.-B., Liu, F.-K., Peng, B., Ma, J., Wu, Z., Jiang, Z. & Chen, J.: Optical monitoring of BL Lacertae object OJ287: A 40 day period? AJ132, 1256-1266 (2006)
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2010
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